One such approach, built up on the dynamical system formulation presented in Sec., was recently introduced by Chakraborty et al [1]}. The formulation employs the same dynamical variables as in Eq.(REF ). Additionally it also makes use of three cosmographic parameters, namely the deceleration, jerk and snap parameters [2]}:
\(q \equiv -\frac{1}{aH^2}\frac{d^2 a}{dt^2}, \qquad j \equiv \frac{1}{aH^3}\frac{d^3 a}{dt^2}, \qquad s \equiv \frac{1}{aH^4}\frac{d^4 a}{dt^2},\) 
